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Temperature in transition region and inner corona

โœ Scribed by Suresh Chandra


Publisher
Springer Netherlands
Year
1983
Tongue
English
Weight
71 KB
Volume
96
Category
Article
ISSN
0004-640X

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๐Ÿ“œ SIMILAR VOLUMES


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The energy balance equation for a general solar atmosphere without assuming the planeparallel approximation is solved analytically. This leads to models for both the transition region and inner corona as well as for the outer corona. The form of the latter is very similar to that of the hydrostatic

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Emission gradient curves for extreme ultraviolet (EUV) resonance lines of O vI and Mg x have been constructed from spectroheliograms of quiet limb regions observed with the Harvard experiment on Skylab. An analysis of these data suggests that the coronal temperature rises throughout the height range